13-16 February 2012
CERN
Europe/Zurich timezone
- conf@2012.uhecr.org
Contact
High Energy Neutrinos from Charm in Astrophysical Sources
Presented by Prof. Ina SARCEVIC
Type: poster
Content
We present results for neutrino fluxes from astrophysical sources.
We show that charm production enhances a flux of very high energy neutrinos from astrophysical sources with jets driven by central engines, such as gamma ray bursts or supernovae with jets. The neutrino flux from semi-leptonic decays of charmed mesons is subject to much less hadronic and radiative cooling than the conventional flux from pion and kaon decays and therefore has a dominant contribution at higher energies, of relevance to future ultrahigh energy neutrino experiments.
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